Published March 1, 2012 | Version v1
Journal article

ANGULAR MOMENTUM CHANGING TRANSITIONS IN PROTON-RYDBERG HYDROGEN ATOM COLLISIONS

  • 1. Department of Physics, Texas Southern University, Houston, TX 77004 (United States)
  • 2. Dipartimento di Fisica e Astronomia 'Galileo Galilei', Università di Padova, 35131 Padova (Italy)
  • 3. ITAMP, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)

Description

Collisions between electrically charged particles and neutral atoms are central for understanding the dynamics of neutral gases and plasmas in a variety of physical situations of terrestrial and astronomical interest. Specifically, redistribution of angular momentum states within the degenerate shell of highly excited Rydberg atoms occurs efficiently in distant collisions with ions. This process is crucial in establishing the validity of the local thermal equilibrium assumption and may also play a role in determining a precise ionization fraction in primordial recombination. We provide an accurate expression for the non-perturbative rate coefficient of collisions between protons and H(nl) ending in a final state H(nl'), with n being the principal quantum number and l, l' the initial and final angular momentum quantum numbers, respectively. The validity of this result is confirmed by results of classical trajectory Monte Carlo simulations. Previous results, obtained by Pengelly and Seaton only for dipole-allowed transitions l → l ± 1, overestimate the l-changing collisional rate coefficients approximately by a factor of six, and the physical origin of this overestimation is discussed.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/747/1/56

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
747
Journal Issue
1
Journal Page Range
[7 p.]
ISSN
0004-637X
CODEN
ASJOAB